Phase curve: Yes Dayside Temperature (occultation): 2900 K |
Spitzer | A Comprehensive Analysis Spitzer 4.5 $μ$m Phase Curve of Hot Jupiters2024, Lisa Dang, Taylor J. Bell et al. |
Dayside and nightside temperatures from phase curve at 4.5 um. Negative albedo |
H2O: Detection FeH: Detection CO2: Detection
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HST WFC3 | Five key exoplanet questions answered via the analysis of 25 hot Jupiter atmospheres in eclipse2022, Quentin Changeat, Billy Edwards et al. |
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Phase curve: Yes |
TESS | Reassessing the Evidence for Time Variability in the Atmosphere of the Exoplanet HAT-P-7 b2022, Maura LallyAndrew Vanderburg |
Supergranulation alone can cause the amplitude and phase offset variability we detect for HAT-P-7 |
Phase curve: Yes |
TESS | Visible-light Phase Curves from the Second Year of the TESS Primary Mission2021, Ian Wong, Daniel Kitzmann et al. |
Significant detections of secondary eclipse (D=127+/-33 ppm) and planetary phase curve modulation. |
Dayside Temperature (occultation): 2692 K |
HST WFC3 | An HST/WFC3 Thermal Emission Spectrum of the Hot Jupiter HAT-P-7b2018, Mansfield, Megan, Bean, Jacob L. et al. |
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Phase curve: Yes |
Spitzer | 3.6 and 4.5 μm Spitzer Phase Curves of the Highly Irradiated Hot Jupiters WASP-19b and HAT-P-7b2016, Wong, Ian, Knutson, Heather A. et al. |
Upper limit on the bond albedo of 0.08 (1σ) |